1980
DOI: 10.1103/physrevb.21.2415
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Dynamics of dense laser-induced plasmas

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Cited by 280 publications
(76 citation statements)
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“…The average absorbed laser energy density is a function of excitation fluence and probe depth. This model is consistent with the expected fast electronic equilibration [24] and compara- tively slow rate of phonon emission [21] and ambipolar diffusion in a dense plasma [25]. In order to compare disordering time scales, the time required for the diffraction intensity to drop to 1=e of its original value ( 1=e ) is used.…”
Section: Institut Für Experimentelle Physik Universität Duisberg-essmentioning
confidence: 63%
“…The average absorbed laser energy density is a function of excitation fluence and probe depth. This model is consistent with the expected fast electronic equilibration [24] and compara- tively slow rate of phonon emission [21] and ambipolar diffusion in a dense plasma [25]. In order to compare disordering time scales, the time required for the diffraction intensity to drop to 1=e of its original value ( 1=e ) is used.…”
Section: Institut Für Experimentelle Physik Universität Duisberg-essmentioning
confidence: 63%
“…The fullest analyses of the non-radiative transitions are those of Yoffa (1980) and Dumke (1980). Both note that Auger recombination is fast at high carrier densities.…”
Section: Laser Annealingmentioning
confidence: 99%
“…22,23 The dynamics of nanosecond-laser heating and the melting threshold are usually described within the frames of the thermal model based on the heat-flow equation. 24,25 At shorter laser pulses, the electron and lattice subsystems are treated separately, involving ambipolar diffusion [26][27][28][29] or drift-diffusion 14,30,31 approaches. By using a drift-diffusion formalism, it has been demonstrated that the macroscopic Coulomb explosion in silicon is improbable at femtosecond, IR laser irradiation, 30 while the conditions for electrostatic disintegration of the external layer of the silicon targets can be created at longer, nanosecond UV pulses 31,32 with fluences below the melting threshold.…”
Section: Introductionmentioning
confidence: 99%